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Fig. 9.
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Details of the (n–σ) plane for higher values of n for several values of cosmological parameter, λ. Depicted is the ratio of the radius ξ1 and the static radius ξs ≡ (3ν(ξ1)/2λ)1/3 for the finite configurations. In the plotted region, all considered configurations are unstable to radial perturbations.
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